The force-free magnetosphere around an oblique rotator

Details The force-free magnetosphere around an oblique rotator The force-free magnetosphere around an oblique rotator

Jun 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998mnras.297..315u&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Volume 297, Issue 1, pp. 315-322.

Astronomy and Astrophysics

Astronomy

2

Mhd, Pulsars: General

Scientific paper

The force-free magnetosphere around an obliquely rotating pulsar is studied. The basic equations reduce to two equations for two Euler potentials. One of the Euler potentials is regarded as a generalization of the stream function of the poloidal magnetic field lines in an axisymmetric rotator. Two divergence-free vectors become tangential to the surface on which this Euler potential is constant.

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